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SMART for the Next Decade

Published online by Cambridge University Press:  13 April 2010

Myung Gyoon Lee ,
In-Soo Yuk  and
Sungsoon Lim
Myung Gyoon Lee
Affiliation:
Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea email: mglee@astro.snu.ac.kr, slim@astro.snu.ac.kr
In-Soo Yuk
Affiliation:
Korea Astronomy and Space Science Institute, Daejeon 305–348, Korea email: yukis@kasi.re.kr
Sungsoon Lim
Affiliation:
Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea email: mglee@astro.snu.ac.kr, slim@astro.snu.ac.kr
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Abstract

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SMART is a model to derive both star formation history and chemical evolution simultaneously from color-magnitude diagrams of resolved stars in a galaxy. We present current progress and discuss the prospects of SMART for the next decade.

Keywords

galaxies: dwarfLocal Groupgalaxies: stellar contentgalaxies: evolution
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S262: Stellar Populations – Planning for the Next Decade , August 2009 , pp. 291 - 294
Copyright
Copyright © International Astronomical Union 2010

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